HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Channel and Crater in Rahway Valles: ESP_069755_1910 ESP_070177_1910 (Interval in Earth days: 33)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
10.90	174.	13.4	-18.2	51.7	54.8
Recent Crater on Northern Plains: ESP_069968_2390 ESP_069889_2390 (Interval in Earth days: 6)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
58.81	110.	9.20	-6.73	50.1	51.9
Fluvial Feature South of Candidate ExoMars Landing Site in Oxia Planum: ESP_069815_1975 ESP_072017_1975 (Interval in Earth days: 171)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.56	335.	10.7	-21.7	49.9	53.3
Undeveloped Collapse Pit: ESP_069849_1975 ESP_070060_1975 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
17.41	127.	7.78	-7.90	50.1	51.5
Mounds in Southern Jezero Crater: ESP_069864_1985 ESP_069930_1985 (Interval in Earth days: 5)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.13	77.5	12.6	-11.4	49.5	51.5
Fractured Crater Floor: ESP_069920_1775 ESP_070131_1775 (Interval in Earth days: 16)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-2.32	351.	5.84	-11.0	58.7	60.4
Mesa in Chryse Planitia: ESP_069644_1990 ESP_069433_1990 (Interval in Earth days: 17)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
18.86	323.	11.6	-6.14	49.0	49.3
Xanthe Dorsa: ESP_069987_2245 ESP_070277_2245 (Interval in Earth days: 23)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
44.03	317.	-7.5	5.319	48.4	46.5
Layering in Arabia Terra: ESP_069656_1845 ESP_069313_1845 (Interval in Earth days: 26)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
4.212	-0.4	-4.1	6.566	55.2	51.5
Impact Crater with Central Peak: ESP_069803_1550 ESP_070449_1550 (Interval in Earth days: 50)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-24.5	310.	-7.2	5.522	71.8	73.3
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